Measured projected 2PCF for full sample and AGN subsamples. The errorbars correspond to 1σ estimated via the bootstrap method. The solid lines show the squared best-fit bias times the projected DM correlation function estimated at the mean redshift of the particular sample. The gray datapoints are not used in the fit due to a low number of pairs. The excess correlation at r_p ∼ 15 h⁻¹ Mpc is likely driven by large structure in the COSMOS field.